HD 111232 b

HD 111232 b is an extrasolar planet that orbits at almost 2 AU with a minimum mass of 6.8 times that of Jupiter. This planet was discovered in the La Silla Observatory by Michel Mayor using the CORALIE spectrograph on 30 June 2003, along with six other planets, including HD 41004 Ab, HD 65216 b, HD 169830 c, HD 216770 b, HD 10647 b, and HD 142415 b.[2]

HD 111232 b
Discovery
Discovered byMayor et al.
Discovery siteLa Silla Observatory, Chile
Discovery date30 June 2003
Doppler Spectroscopy
(CORALIE)
Orbital characteristics[1]
2.148+0.088
−0.097 AU
Eccentricity0.214+0.005
−0.003
3.201+0.002
−0.001 yr
Inclination93.521°+16.622°
−18.063°
358.306°+52.528°
−32.102°
2452361.045+4.144
−3.497
94.142°+0.920°
−0.719°
Semi-amplitude160.429+0.573
−0.509 m/s
StarHD 111232
Physical characteristics[1]
Mass7.965+1.128
−0.479 MJ

    An astrometric measurement of the planet's inclination and true mass was published in 2022 as part of Gaia DR3.[3]

    References
    1. Feng, Fabo; Butler, R. Paul; et al. (August 2022). "3D Selection of 167 Substellar Companions to Nearby Stars". The Astrophysical Journal Supplement Series. 262 (21): 21. arXiv:2208.12720. Bibcode:2022ApJS..262...21F. doi:10.3847/1538-4365/ac7e57. S2CID 251864022.
    2. Mayor, M.; et al. (2004). "The CORALIE survey for southern extra-solar planets XII. Orbital solutions for 16 extra-solar planets discovered with CORALIE". Astronomy and Astrophysics. 415 (1): 391–402. arXiv:astro-ph/0310316. Bibcode:2004A&A...415..391M. doi:10.1051/0004-6361:20034250. S2CID 5233877.
    3. Gaia Collaboration; et al. (2022). "Gaia Data Release 3: Stellar multiplicity, a teaser for the hidden treasure". arXiv:2206.05595 [astro-ph.SR].
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